High-Energy Measurements of the November 15, 1991 Solar Flare

Details High-Energy Measurements of the November 15, 1991 Solar Flare High-Energy Measurements of the November 15, 1991 Solar Flare

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mwoc.conf..397r&link_type=abstract

Multi-Wavelength Observations of Coronal Structure and Dynamics -- Yohkoh 10th Anniversary Meeting. Proceedings of the conferenc

Computer Science

Scientific paper

This event was well observed by Yohkoh, Compton and ground-based observatories. Gamma rays were detected up to 8 MeV indicative of an accelerated ion spectrum containing at least 1027 ergs with a spectrum of E(-4.5). This amount of energy is not sufficient to produce the detected white light emission. The ions also produced neutrons that in turn generated 2.223 MeV gamma-ray emission. The time decay of this emission is unusually rapid (26 s) suggesting an elevated abundance of 3He assuming the absence of much higher energy particles.

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